Okay, so we're starting with d = rt. "Distance equals rate times time." If you divide both sides by t, you would get r = d/t. So, your answer is A. Another explanation: let's say you've traveled 120 miles in 2 hours. How fast were you going? To solve that, you would divide your distance (120) by your time (2) to get 60 mph. So, rate = distance/time.Hope this helps.
the picture that shows a plain is 4
Answer:
pluto, neptune, Uranus, and jupiter
hope this helps :)
Explanation:
When it is noon in Massena, New York, it would be 5PM in Greenwich, England. Why? Because the time zone in Massena is UTC -5, meaning that it is behind by 5 hours. Greenwich, England is UTC 0, so when it’s noon in Massena, New York, it would be 5PM.
It depends on the latitude where you measure it.
It's about 69 miles on the equator, and it shrinks to zero at the poles.
In general, at any latitude,
Distance covered by 1 degree of longitude =
<em> (69 miles) x [ cosine(latitude where it's measured) ]</em>
